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2018 | OriginalPaper | Chapter

Numerical Simulation of Circumsolar Ring Evolution

Authors: A. S. Murachev, D. V. Tsvetkov, E. M. Galimov, A. M. Krivtsov

Published in: Advances in Mechanics of Microstructured Media and Structures

Publisher: Springer International Publishing

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Abstract

The results of the computer simulation for the circumsolar gas-dust cloud evolution are presented. The particle dynamics method is used. We show that gas-dust clusters can be formed in ring-shaped structures of protoplanetary disks. It is demonstrated that the clusters are formed as a result of the counteracting of the self-gravitational force of the ring and the gravity of the Sun. This process has a probabilistic nature. The range of the system parameters providing the clusters formation is obtained. Different scenarios of the ring evolution are observed and analyzed. The considered gas-dust clusters can be precursors for the further formation of the planet-satellite systems.

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Metadata
Title
Numerical Simulation of Circumsolar Ring Evolution
Authors
A. S. Murachev
D. V. Tsvetkov
E. M. Galimov
A. M. Krivtsov
Copyright Year
2018
DOI
https://doi.org/10.1007/978-3-319-73694-5_14

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